Arrival of plasmas, particles and electromagnetic radiation decide the ... D. Webb (USA, IAU Rep. ) S. T. Wu (USA) M. Kojima (Japan) M. Zhang (China) Objectives ...
Focus on two specific kinds of CME progenitors: erupting filaments and coronal sigmoids ... Webb (p.c.), Jones (p.c.) Collect solar wind data from ACE, Wind ...
Focusing on the features of the sun (photosphere and corona) 8/23 24 25 26 27. Dst Index ... twisted magnetic structure lies beneath the photosphere! ...
Figure 6 (Movie): But the solar signatures in Yohkoh/SXT images around the ... Figure 12 (Movie) : TRACE example of 'unsuccessful ejection', not leading to a CME. ...
Extreme Solar Activity of Oct 2003. Disturbed Chemisty. Deep Ionization ... http://www.ee.surrey.ac.uk/Personal/L.Wood/constellations/iridium.html. Iridium ...
... (calibration, compression, remapping) at GONG sites, established near-real ... of the farside images and will place them at http://gong.nso.edu/data/farside. ...
Title: Slide 1 Author: Elena Last modified by: EV Created Date: 11/13/2006 9:49:20 PM Document presentation format: On-screen Show Company: Royal Observatory of Belgium
... at solstice but developed into a two-stream, four-sector pattern at equinox. ... Coleman effect arises because at equinox the Earth is immersed longer in ...
More about flows in Poster previews! Modelers using these data to simulate eruptions! ... (BACK) Petrinec et al. (1998) Movie of Bow Shock, Magnetopause (BACK) ...
The follow-up science meeting was held 1-year after the CDAW. ... For the scientific output, follow-up science meeting and solid publication plan are important. ...
NASA Goddard Space Flight Center, Greenbelt, Maryland ... apex with solar North. Width = PA2 PA1. Speed = dh/dt. W. S. N. PA1. PA2. CPA (h,t) Height-Time Plot ...
loop strands with isothermal cross-sections, at FWHM widths of ... in the CELTIC model is consistent. with a semi-Gaussian distribution. with a Gaussian width of ...
Halo coronal mass ejections and proton events during ... SOHO/ERNE proton intensities. 1.8 - 80 MeV in six energy channels. Storm Sudden Commencement (SSC) ...
(Catholic University of America) R. A. Howard (Naval Research Laboratory) ... to the Sun-Observer line (majority backside) selection effect (occultation) ...
Hannu Koskinen (1,2), Tuomo Nygren (3), Risto ... (1) University of Helsinki, Department of Physical Sciences ... coronagraph observations. imaging intsruments. ...
Using real-time solar wind data from the ACE spacecraft as input to a filter, e. ... between geomagnetic activity and the boundaries between low-speed and high-speed ...
Stanford solar group is a member of CISM (It is a NSF's Science and Technology ... orientation of rope-like structures for the 3 CMEs using the ZEC; and thirdly ...
... T.I., De Zeeuw, D.L., Groth, C.P.T., Powell, K.G, C. Robert Clauer, and Paul ... By Song P., H. J. Singer, and G. L. Siscoe, Geophysical Monograph 125, AGU ...
Emission is seen from top of the band (14 MHz) down to ~ 8 MHz and at ~ 14:05-15: ... a bewildering complex of many narrow-band emissions drifting downward from ~ 3-1 ...
F2B: Quantify Particle Acceleration for Key Regions of Exploration ... Dipper mission, Earth analog to dynamics and variability of the lower thermosphere ...
European Space Weather Modelling Activities: A look at Current Capabilities and the Transition to Operational Services A Glover1,2, A Hilgers1, E Daly1, A Belehaki3
3-d viewer or some way to display what's coming at us on the Sun-Earth line. SECCHI team ... Includes near-Earth (ACE) data sets for third point views & image ...
Sigmoid Detection Problems. Structure and intensity not well correlated ... Test results: sigmoid detector successfully flags periods of high activity ...
... Multidisciplinary University Research Initiative Team. UC Berkeley ... UC San Diego. University of Colorado. University of Hawaii. University of New Hampshire ...
The Geoeffectiveness of Solar Cycle 23. as inferred from a Physics-Based Storm Model ... interplanetary conditions on energetic particle dynamics and how large ...
Infra-red lines formed in solar corona can be used to measure magnetic fields. ... in Ha of a classic 2-ribbon flare, taken by Johns-Krull and Fisher ...
Understanding Magnetic Eruptions on the Sun and their Interplanetary Consequences ... flow should have non-zero vorticity, to ensure some component of magnetic ...
The fundamental importance of the penetration electric field for the dynamical ... Penetration fields persist for longer periods because stretched field ...
The temperature of hot-ions at geosynchronous orbit vary with time and local ... UT-LT Maps: Color-coded Geosynchronous Observations. White Bins: No Data Available; ...
... the Sun (part of the corona is expelled with its magnetic field) ... corona ... modern sense (OSO-7): Tousey, R., The solar corona, Adv. Space Res., 13,713, 1973. ...
... tools and projects below shows the kind of ideas being ... van der Linden ROB Uses fast internet access & caching. ... SWAVES teams UCLA radio data from STEREO. ...
The STEREO Space Weather Group consists of scientists associated with the STEREO ... JAVA-3D Synoptic J. Luhmann, P. Schroeder JAVA-3D applet for viewing 3D Sun ...
Can we infer the orientation of Bz of an ICME at 1 AU by focusing on the study ... A. Nindos: Examined chirality of source region using photospheric magnetograms ...